Cargando…
Light higgsino detection at LEP1.5
Within the minimal supersymmetric extension of the Standard Model, the best fit to the most recent precision-measurement data requires charginos and neutralinos, with dominant Higgsino components and with masses within the reach of LEP1.5 (\sqrt{s}=140 GeV). In this work, we present a detailed analy...
Autores principales: | , , , |
---|---|
Lenguaje: | eng |
Publicado: |
1995
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/0370-2693(96)00129-3 http://cds.cern.ch/record/290952 |
_version_ | 1780888620889014272 |
---|---|
author | Ambrosanio, S. Mele, B. Carena, Marcela Wagner, C.E.M. |
author_facet | Ambrosanio, S. Mele, B. Carena, Marcela Wagner, C.E.M. |
author_sort | Ambrosanio, S. |
collection | CERN |
description | Within the minimal supersymmetric extension of the Standard Model, the best fit to the most recent precision-measurement data requires charginos and neutralinos, with dominant Higgsino components and with masses within the reach of LEP1.5 (\sqrt{s}=140 GeV). In this work, we present a detailed analysis of the neutralino and chargino production processes for the favoured region of parameter space, that is low values of |\mu| and either low or large values of \tan\beta. We find that chargino and neutralino searches can cover the Higgsino region in the (\mu,M_2) plane for values of M_2 \simlt 1~TeV, at the next phases of the LEP collider. We also show that, due mainly to phase-space constraints, the lightest neutralinos should be more easily detectable than charginos in most of the parameter space preferred by precision-measurement data. |
id | cern-290952 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1995 |
record_format | invenio |
spelling | cern-2909522023-03-14T19:55:49Zdoi:10.1016/0370-2693(96)00129-3http://cds.cern.ch/record/290952engAmbrosanio, S.Mele, B.Carena, MarcelaWagner, C.E.M.Light higgsino detection at LEP1.5Particle Physics - PhenomenologyWithin the minimal supersymmetric extension of the Standard Model, the best fit to the most recent precision-measurement data requires charginos and neutralinos, with dominant Higgsino components and with masses within the reach of LEP1.5 (\sqrt{s}=140 GeV). In this work, we present a detailed analysis of the neutralino and chargino production processes for the favoured region of parameter space, that is low values of |\mu| and either low or large values of \tan\beta. We find that chargino and neutralino searches can cover the Higgsino region in the (\mu,M_2) plane for values of M_2 \simlt 1~TeV, at the next phases of the LEP collider. We also show that, due mainly to phase-space constraints, the lightest neutralinos should be more easily detectable than charginos in most of the parameter space preferred by precision-measurement data.Within the minimal supersymmetric extension of the Standard Model, the best fit to the most recent precision-measurement data requires charginos and neutralinos, with dominant Higgsino components and with masses within the reach of LEP1.5 ($\sqrt{s}=140$ GeV). In this work, we present a detailed analysis of the neutralino and chargino production processes for the favoured region of parameter space, that is low values of $|\mu|$ and either low or large values of $\tan\beta$. We find that chargino and neutralino searches can cover the Higgsino region in the ($\mu,M_2$) plane for values of $M_2 \simlt 1$TeV, at the next phases of the LEP collider. We also show that, due mainly to phase-space constraints, the lightest neutralinos should be more easily detectable than charginos in most of the parameter space preferred by precision-measurement data.Within the minimal supersymmetric extension of the Standard Model, the best fit to the most recent precision-measurement data requires charginos and neutralinos, with dominant Higgsino components and with masses within the reach of LEP1.5 ( S =140 GeV ). In this work, we present a detailed analysis of the neutralino and chargino production processes for the favoured region of parameter space, that is low values of |μ| and either low or large values of tan β. We find that chargino and neutralino searches can cover the Higgsino region in the (μ, M 2 ) plane for values of M 2 ≲ 1 TeV, at the next phases of the LEP collider. We also show that, due mainly to phase-space constraints, the lightest neutralinos should be more easily detectable than charginos in most of the parameter space preferred by precision-measurement data.hep-ph/9511259CERN-TH-95-286ROME1-1121-95CERN-TH-95-286ROMA-1-1121oai:cds.cern.ch:2909521995-11-07 |
spellingShingle | Particle Physics - Phenomenology Ambrosanio, S. Mele, B. Carena, Marcela Wagner, C.E.M. Light higgsino detection at LEP1.5 |
title | Light higgsino detection at LEP1.5 |
title_full | Light higgsino detection at LEP1.5 |
title_fullStr | Light higgsino detection at LEP1.5 |
title_full_unstemmed | Light higgsino detection at LEP1.5 |
title_short | Light higgsino detection at LEP1.5 |
title_sort | light higgsino detection at lep1.5 |
topic | Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1016/0370-2693(96)00129-3 http://cds.cern.ch/record/290952 |
work_keys_str_mv | AT ambrosanios lighthiggsinodetectionatlep15 AT meleb lighthiggsinodetectionatlep15 AT carenamarcela lighthiggsinodetectionatlep15 AT wagnercem lighthiggsinodetectionatlep15 |